{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:PHLQSXZWT3S7DGFVZJKBGDKDZD","short_pith_number":"pith:PHLQSXZW","schema_version":"1.0","canonical_sha256":"79d7095f369ee5f198b5ca54130d43c8fc4226a61890be2dd177a522dbc870b8","source":{"kind":"arxiv","id":"1407.4572","version":3},"attestation_state":"computed","paper":{"title":"Irradiation of Nuclear Track Emulsions with Thermal Neutrons, Heavy Ions, and Muons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. A. Zaitsev, D.A. Artemenkov, I. G. Zarubina, K. Z. Mamatkulov, P. I. Zarubin, R. R. Kattabekov, V. Bradnova, V. V. Rusakova","submitted_at":"2014-07-17T06:17:59Z","abstract_excerpt":"Exposures of test samples of nuclear track emulsion were analyzed. Angular and energy correlations of products originating from the thermal-neutron-induced reaction n$_{th} + ^{10}$B $\\rightarrow ^{7}$Li $+ (\\gamma) + \\alpha$ were studied in nuclear tack emulsions enriched in boron. Nuclear track emulsions were also irradiated with $^{86}$Kr$^{+17}$ and $^{132}$Xe$^{+26}$ of energy about 1.2 MeV per nucleon. Measurements of ranges of heavy ions in nuclear track emulsions made it possible to determine their energies on the basis of the SRIM model. The formation of high-multiplicity nuclear star"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1407.4572","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2014-07-17T06:17:59Z","cross_cats_sorted":[],"title_canon_sha256":"8655c68b0c102d1782be0a4b1e153d7fc4936dbc25f102c5171f3d967c80921d","abstract_canon_sha256":"f5d7f2c469a2c4fc810481888cf0b792eeaf85ad413b84096cc13da432774bc4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:32.923149Z","signature_b64":"sKucQuiKedxv8fIY7zjFxMNHpJIFJh4PoeCd9UEtka9cRA98SHstGkhaEk/M67ur0vKXUiyxqO6CYjuE+Y4lBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"79d7095f369ee5f198b5ca54130d43c8fc4226a61890be2dd177a522dbc870b8","last_reissued_at":"2026-05-18T01:35:32.922605Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:32.922605Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Irradiation of Nuclear Track Emulsions with Thermal Neutrons, Heavy Ions, and Muons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. A. Zaitsev, D.A. Artemenkov, I. G. Zarubina, K. Z. Mamatkulov, P. I. Zarubin, R. R. Kattabekov, V. Bradnova, V. V. Rusakova","submitted_at":"2014-07-17T06:17:59Z","abstract_excerpt":"Exposures of test samples of nuclear track emulsion were analyzed. Angular and energy correlations of products originating from the thermal-neutron-induced reaction n$_{th} + ^{10}$B $\\rightarrow ^{7}$Li $+ (\\gamma) + \\alpha$ were studied in nuclear tack emulsions enriched in boron. Nuclear track emulsions were also irradiated with $^{86}$Kr$^{+17}$ and $^{132}$Xe$^{+26}$ of energy about 1.2 MeV per nucleon. Measurements of ranges of heavy ions in nuclear track emulsions made it possible to determine their energies on the basis of the SRIM model. The formation of high-multiplicity nuclear star"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.4572","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1407.4572","created_at":"2026-05-18T01:35:32.922687+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.4572v3","created_at":"2026-05-18T01:35:32.922687+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.4572","created_at":"2026-05-18T01:35:32.922687+00:00"},{"alias_kind":"pith_short_12","alias_value":"PHLQSXZWT3S7","created_at":"2026-05-18T12:28:43.426989+00:00"},{"alias_kind":"pith_short_16","alias_value":"PHLQSXZWT3S7DGFV","created_at":"2026-05-18T12:28:43.426989+00:00"},{"alias_kind":"pith_short_8","alias_value":"PHLQSXZW","created_at":"2026-05-18T12:28:43.426989+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2601.21425","citing_title":"The $^{8}$Be nucleus and the Hoyle state in dissociation of relativistic nuclei","ref_index":36,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD","json":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD.json","graph_json":"https://pith.science/api/pith-number/PHLQSXZWT3S7DGFVZJKBGDKDZD/graph.json","events_json":"https://pith.science/api/pith-number/PHLQSXZWT3S7DGFVZJKBGDKDZD/events.json","paper":"https://pith.science/paper/PHLQSXZW"},"agent_actions":{"view_html":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD","download_json":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD.json","view_paper":"https://pith.science/paper/PHLQSXZW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.4572&json=true","fetch_graph":"https://pith.science/api/pith-number/PHLQSXZWT3S7DGFVZJKBGDKDZD/graph.json","fetch_events":"https://pith.science/api/pith-number/PHLQSXZWT3S7DGFVZJKBGDKDZD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD/action/storage_attestation","attest_author":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD/action/author_attestation","sign_citation":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD/action/citation_signature","submit_replication":"https://pith.science/pith/PHLQSXZWT3S7DGFVZJKBGDKDZD/action/replication_record"}},"created_at":"2026-05-18T01:35:32.922687+00:00","updated_at":"2026-05-18T01:35:32.922687+00:00"}